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Home All issues Volume 508 / No 1 (December II 2009) A&A, 508 1 (2009) 531-539 Full HTML
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Table 3:

Values of $\langle g^{(2)}(d) \rangle$ obtained from one hour observation of the bright star $\zeta $ Ori, for each pair a,bof sub-apertures, assuming a time coincidence window $\Delta t = 244.1$ ps.
Channel pair Effective distance Resolving angle $\langle g^{(2)}(d) \rangle$ Standard
(channel numbers) d (m) $\theta$ (arcsec)   deviation
A-B 1.7 0.052 0.886 0.002
A-C 2.4 0.037 0.912 0.003
A-D 1.7 0.052 0.931 0.001
B-C 1.7 0.052 0.909 0.002
B-D 2.4 0.037 0.909 0.004
C-D 1.7 0.052 0.932 0.004


Source LaTeX | All tables | In the text

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